We have investigated GR and EQG prediction for GL effects by some SMBHs in our galaxy and other thirteen galaxies. By considering the Sgr A* as the lens and EQG coupling constant as \(K = 8.98 \times 10^{38} M_{}^4\) , for which EQG passes all Solar System tests to date [1]}, we calculated the angular positions of primary and secondary images deviation from that of GR by an amount of order of miliarcseconds. As well, using numerical methods we have generally shown that the EQG results for the differential time delay, associated with primary and secondary images, could be some tenths of seconds shorter than the results of GR for a lots of number of \(\beta \)  (please see Fig. REF ).
